Fig. 3.
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Kinetic luminosity density of (radio) AGN as a function of redshift obtained from recent observational work. Results of this work are shown by the thick black cross. The yellow shaded region also shows the 0.1 − 1% of bolometric luminosity density from Aird et al. (2015) which represents a rough indicator of the ‘canonical’ feedback energy that may be delivered by radiatively driven AGN winds.
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